Tracing the evolution of high-mass stars: combining maser evolutionary timelines with chemical clocks

追踪大质量恒星的演化：将微波激射器演化时间线与化学钟相结合

• 批准号: DE130101270
• 负责人: Dr Shari Breen
• 金额: $ 23.4万
• 依托单位: Commonwealth Scientific and Industrial Research Organisation
• 依托单位国家: 澳大利亚
• 项目类别: Discovery Early Career Researcher Award
• 财政年份: 2013
• 资助国家: 澳大利亚
• 起止时间: 2013-06-30 至 2016-06-25
• 项目状态: 已结题
• 来源: https://dataportal.arc.gov.au/RGS/Web/Grants/DE130101270
• 关键词: Tracing; evolution; mass; stars; combining

Maser emission (radio analogue of lasers) arises naturally in the dense gas surrounding young, large stars. Studying many types of masers towards lots of sources will allow us to uncover the precise stages of star formation that each maser species is tracing. Such a timeline promises to be an important tool in determining how these big stars form.

脉泽发射（激光的无线电模拟）在年轻的大恒星周围的致密气体中自然产生。研究多种类型的脉泽，将使我们能够揭示每种脉泽所追踪的星星形成的精确阶段。这样的时间轴有望成为确定这些大恒星如何形成的重要工具。